Binary star systems in Camelopardalis

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                                             Binary star systems in Camelopardalis

 The most massive known binary star systems by astronomers in Camelopardalis. The system consists of two hot blue O-type stars orbiting very close to each other with a period of 1.2 days. Scientists at the University of Alicante hope that by seeing the merger of binary stars so the event could reveal,for the first time, how super massive stars are born the eclipsing of a star system, that observations suggest, of today astronomers by looking at the high-resolution of the two stars with the powerful 2.2-meter telescope at the Calar Alto Observatory in southern Spain, in order to explain this light are called spectrographs are very usual among the display of instruments equipping all modern observatories.

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